Laser Cooling 1. Doppler Cooling – optical molasses. 2. Magneto-optical trap. 3. Doppler temperature.

Slides:



Advertisements
Similar presentations
Creating new states of matter:
Advertisements

Bose-Einstein Condensation Ultracold Quantum Coherent Gases.
Ultracold Quantum Gases Part 1: Bose-condensed Gases The experimentalist’s perspective Ultracold Quantum Gases Part 1: Bose-condensed Gases The experimentalist’s.
Ultracold Quantum Gases Part 1: Bose-condensed Gases The experimentalist’s perspective Ultracold Quantum Gases Part 1: Bose-condensed Gases The experimentalist’s.
AA and Atomic Fluorescence Spectroscopy Chapter 9
The Bose-Einstein Condensate Jim Fung Phys 4D Jim Fung Phys 4D.
Laser cooling of molecules. 2 Why laser cooling (usually) fails for molecules Laser cooling relies on repeated absorption – spontaneous-emission events.
Compton Effect 1923 Compton performed an experiment which supported this idea directed a beam of x-rays of wavelength  onto a carbon target x-rays are.
Laser Cooling: Background Information The Doppler Effect Two observes moving relative to each other will observe the same wave with different frequency.
Bose-Einstein Condensates Brian Krausz Apr. 19 th, 2005.
Spectrum from a Prism. Example of a Spectrum Kirchoff’s Laws.
Zeeman Slowing W. Phillips, H. Metcalf PRL 48 p569 (1982)
Precision α Measurement: Atom Recoil Method Review Victor Acosta Physics 250: Atomic Physics Prof. Dima Budker.
A Magneto-Optical Trap for Strontium James Millen A Magneto-Optical Trap for Strontium – Group meeting 29/09/08.
Sisyphus Cooling Justin M. Brown November 8, 2007.
P460 - atoms III1 More Energy Levels in Atoms If all (both) electrons are at the same n. Use Hund’s Rules (in order of importance) minimize ee repulsion.
Photons of Light The smallest unit of light is a photon A photon is often called a particle of light The Energy of an individual photon depends on its.
Ultra-Cold Matter Technology Physics and Applications Seth A. M. Aubin University of Toronto, Canada June 15, 2006 NRC, Ottawa.
Quantum Computation Using Optical Lattices Ben Zaks Victor Acosta Physics 191 Prof. Whaley UC-Berkeley.
LECTURE 6, SEPTEMBER 9, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT 1ASTR 101-3, FALL 2010.
Laser Locking for Long-term Magneto-Optical Trap Stability Kevin W. Vogel Advisor: Georg Raithel Presented 07/28/04.
Lecture II Non dissipative traps Evaporative cooling Bose-Einstein condensation.
Light and Matter Tim Freegarde School of Physics & Astronomy University of Southampton Controlling matter with light.
On the path to Bose-Einstein condensate (BEC) Basic concepts for achieving temperatures below 1 μK Author: Peter Ferjančič Mentors: Denis Arčon and Peter.
H. J. Metcalf, P. Straten, Laser Cooling and Trapping.
Colleen Downs Stephanie Pietromonaco Sanjay Talluri
Mössbauer spectroscopy References: J.P. Adloff, R. Guillaumont: Fundamentals of Radiochemistry, CRC Press, Boca Raton, 1993.
Chad Orzel Union College Physics Radioactive Background Evaluation by Atom Counting C. Orzel Union College Dept. of Physics and Astronomy D. N. McKinsey.
Comparison of Methods to Load a Mirror Magneto-Optical Trap Date: 14 May 2009 Author: C. Erin Savell Advisors: Dr. Shaffer and Arne Schwettmann Acknowledgement:
Determination of fundamental constants using laser cooled molecular ions.
Module 1: Atomic and molecular physics, 10 lectures, Ben Sauer Collision physics at low temperature, 4 lectures, Misha Ivanov Module 2: Laser cooling and.
Theoretical Study of the Optical Manipulation of Semiconductor Nanoparticles under an Excitonic Resonance Condition + Reference + T.Iida and H.Ishihara,
High-performance Apparatus for Bose-Einstein Condensation of Rubidium Yoshio Torii Erik Streed Micah Boyd Gretchen Campbell Pavel Gorelik Dominik Schneble.
Quantum Physics & Ultra-Cold Matter Seth A. M. Aubin Dept. of Physics College of William and Mary December 16, 2009 Washington, DC.
Light and Matter Astronomy 315 Professor Lee Carkner Lecture 6.
Can we build individual molecules atom by atom? Mikkel F. Andersen Jack Dodd Centre for Quantum Technology, Department of Physics, University of Otago.
Obtaining Ion and Electron Beams From a source of Laser-Cooled Atoms Alexa Parker, Gosforth Academy  Project Supervisor: Dr Kevin Weatherill Department.
Simple Atom, Extreme Nucleus: Laser Trapping and Probing of He-8 Zheng-Tian Lu Argonne National Laboratory University of Chicago Funding: DOE, Office of.
Light-induced instabilities in large magneto-optical traps G. Labeyrie, F. Michaud, G.L. Gattobigio, R. Kaiser Institut Non Linéaire de Nice, Sophia Antipolis,
Light scattering and atom amplification in a Bose- Einstein condensate March 25, 2004 Yoshio Torii Institute of Physics, University of Tokyo, Komaba Workshop.
Quantum interference phenomenon Quantum interference phenomenon in the cold atomic cascade system $$ : National Science Council and National Space Program.
Refractive Index Enhancement without Absorption N. A. Proite, J. P. Sheehan, J. T. Green, D. E. Sikes, B. E. Unks, and D. D. Yavuz University of Wisconsin,
Chapter 8 An Introduction to Optical Atomic Spectrometry 1
Physics 551 Presentation: Doppler Cooling Zane Shi Princeton University November 6 th, 2007.
Relativistic Quantum Theory of Microwave and Optical Atomic Clocks
What is light? Light can act either like a wave or like a particle Particles of light are called photons.
Possible measurement of electron EDM in atoms with spatially alternating electric field T. Haseyama RIKEN, Japan ( The Institute of Physical and Chemical.
Bose-Einstein Condensation (a tutorial) Melinda Kellogg Wyatt Technology Corporation Santa Barbara, CA June 8, 2010.
Laser Cooling and Trapping Magneto-Optical Traps (MOTs) Far Off Resonant Traps (FORTs) Nicholas Proite.
Duke University, Physics Department and the Fitzpatrick Institute for Photonics · Durham, NC Collective Nonlinear Optical Effects in an Ultracold Thermal.
Trap laser (6 mW - 1 cm diameter) x 6 -  /2 detuned to 171Yb 1P1 oven Zeeman slower Trapped atom number Lens f=7.5 cm, diameter d=2.54 cm PMT = 5
Chapter 11. Laser Oscillation : Power and Frequency
Chapter 9 Laser cooling and trapping
Jerzy Zachorowski M. Smoluchowski Institute of Physics, Jagiellonian University Nonlinear Spectroscopy of Cold Atoms, Preparations for the BEC Experiments.
§3.3 Optical Resonators with Spherical Mirrors We will show the field solutions inside the spherical mirror resonator are Gaussian Beams Z=0 00 z R2R2.
Investigation of the Saturation Mechanism of Recoil-induced Resonances Joel A. Greenberg, Marcos Oria, and Daniel J. Gauthier Duke University 5/28/2008.
Ultracold Quantum Gases Part 1 Making and Probing Bose-condensed Gases Ultracold Quantum Gases Part 1 Making and Probing Bose-condensed Gases TexPoint.
Laser Cooling and Trapping
Laser Cooling and Trapping
7. Ideal Bose Systems Thermodynamic Behavior of an Ideal Bose Gas
Making cold molecules from cold atoms
Dan Mickelson Supervisor: Brett D. DePaola
5-level Rabi-flopping Rabi-flopping of a 5-level Zeeman split atom:
Lasers and effects of magnetic field
A New Design for a Tunable External Cavity Diode Laser
Laser Locking for Long-term Magneto-Optical Trap Stability
Quantum Mechanical View of Atoms
7. Ideal Bose Systems Thermodynamic Behavior of an Ideal Bose Gas
Accelerator Physics NMI and Synchrotron Radiation
Cold Atom project 12/02/2019.
Presentation transcript:

Laser Cooling 1. Doppler Cooling – optical molasses. 2. Magneto-optical trap. 3. Doppler temperature.

Doppler Cooling: How can a laser cool? Lab frame v 

v  Atom’s frame Doppler Cooling: How can a laser cool?

Lab frame v  Atom’s frame Lab frame, after absorption v-v recoil Doppler Cooling: How can a laser cool?

Lab frame v  Atom’s frame Lab frame, after absorption v-v recoil Doppler Cooling: How can a laser cool?

Lab frame v  Atom’s frame  Absorb a photon  atom gets momentum kick.  Repeat process at 10 7 kicks/s  large deceleration.  Emitted photons are radiated symmetrically  do not affect motion on average  Absorb a photon  atom gets momentum kick.  Repeat process at 10 7 kicks/s  large deceleration.  Emitted photons are radiated symmetrically  do not affect motion on average Lab frame, after absorption v-v recoil Doppler Cooling: How can a laser cool?

Lab frame v  Atom’s frame  Absorb a photon  atom gets momentum kick.  Repeat process at 10 7 kicks/s  large deceleration.  Emitted photons are radiated symmetrically  do not affect motion on average  Absorb a photon  atom gets momentum kick.  Repeat process at 10 7 kicks/s  large deceleration.  Emitted photons are radiated symmetrically  do not affect motion on average Lab frame, after absorption v-v recoil m/s m/s 2 87 Rb:  = -  I = I sat V doppler ~ 10 cm/s V recoil = 6 mm/s Doppler Cooling: How can a laser cool?

Magneto-Optical Trap (MOT) Problem: Doppler cooling reduces momentum spread of atoms only.  Similar to a damping or friction force (optical molasses).  Does not reduce spatial spread.  Does not confine the atoms.

Magneto-Optical Trap (MOT) Solution: Spatially tune the laser-atom detuning with the Zeeman shift from a spatially varying magnetic field. z B,  ~10 G/cm ~14 MHz/cm Problem: Doppler cooling reduces momentum spread of atoms only.  Similar to a damping or friction force (optical molasses).  Does not reduce spatial spread.  Does not confine the atoms.

Magneto-Optical Trap E ee gg 2-level atom 

E ee gg magnetic gradient +  z B Magneto-Optical Trap

 E ee gg 4-level atom |g   “F=0”, |e   “F=1” 4-level atom |g   “F=0”, |e   “F=1” magnetic gradient + z m F =0 m F =-1 m F =+1 B Magneto-Optical Trap

 E ee gg 4-level atom |g   “F=0”, |e   “F=1” 4-level atom |g   “F=0”, |e   “F=1” magnetic gradient + m F =0 m F =-1 m F =+1 z B Magneto-Optical Trap

 E ee gg 4-level atom |g   “F=0”, |e   “F=1” 4-level atom |g   “F=0”, |e   “F=1” magnetic gradient + m F =0 m F =-1 m F =+1   z B Magneto-Optical Trap

 E ee gg 4-level atom |g   “F=0”, |e   “F=1” 4-level atom |g   “F=0”, |e   “F=1” magnetic gradient + m F =0 m F =-1 m F =+1   z B -- ++ Magneto-Optical Trap

 E ee gg 4-level atom |g   “F=0”, |e   “F=1” 4-level atom |g   “F=0”, |e   “F=1” magnetic gradient + m F =0 m F =-1 m F =+1   z B -- ++ Magneto-Optical Trap

Magneto-Optical Trap (MOT)

~ 100  K

Magneto-Optical Trap (MOT)

Rb atoms

Francium MOT PROBLEM: Accelerator produces only 10 6 Fr atoms/s.  Very difficult to work with. SOLUTION: SOLUTION: Attach a Francium Magneto-Optical Trap to the accelerator.  Cold Francium is concentrated in ~1 mm 3 volume.  With T < 100  K, Doppler broadening is negligible.  Long integration times.  Minimally perturbative environment (substrate free).

Francium MOT PROBLEM: Accelerator produces only 10 6 Fr atoms/s.  Very difficult to work with. SOLUTION: SOLUTION: Attach a Francium Magneto-Optical Trap to the accelerator.  Cold Francium is concentrated in ~1 mm 3 volume.  With T < 100  K, Doppler broadening is negligible.  Long integration times.  Minimally perturbative environment (substrate free). MOT with ~ Fr atoms MOT collection efficiency ~ 1 %